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Observations of H β and [O III] λ4959 + 5007 Å emission line variability in the spectrum of the NGC 1275 galaxy nucleus observed at AZT-11 telescope in 1982-1987

N. I. Merkulova, D. P. Metik, I. I. Pronik

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Key concepts: Physics, Galaxy, Doubly ionized oxygen, Astrophysics, Telescope, Emission spectrum, Astronomy, Line (geometry)

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Observations of H β and [O III] λ4959 + 5007 Å emission line variability in the spectrum of the NGC 1275 galaxy nucleus observed at AZT-11 telescope in 1982-1987 — Research Paper | ScholarLens